NGC 2012 is a bright emission nebula located in the constellation of Lepus. It is part of a larger star-forming region and is approximately 1,500 light-years away from Earth. The nebula is known for its vivid colors, primarily due to the ionization of hydrogen gas by nearby hot stars. This nebula is often studied by astronomers to understand the processes of star formation and the dynamics of interstellar gas. NGC 2012 is also associated with the Lepus constellation, which contains several other notable celestial objects, making it a point of interest for both amateur and professional astronomers.